PI: Daniel Kennefick · University of Arkansas at Fayetteville
We are running codes to model gravitational waves from sources relevant to the LISA mission (Laser Interferometer Space Antenna), specifically from extreme-mass ratio (EMRI) black hole binaries and coincident galactic binaries (especially white dwarf binaries in the Milky Way). The EMRI code aims to provide detailed information for ultimate use in LISA Data Analysis. The Galactic Binary aspect of the project aims to develop ways to deal with confusion between similar signals that occur at the same time and are visible simultaneously by the LISA detector.
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